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Emission Channels from Perturbed Quantum Black Holes
We calculate the emission of gravitational waves, gravitons, photons, and neutrinos from a perturbed Schwarzschild black hole (BH). The perturbation can be due to either classical or quantum sources and therefore the injected energy can be either positive or negative. The emission can be classical i...
Autores principales: | Brustein, Ram, Sherf, Yotam |
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Lenguaje: | eng |
Publicado: |
2019
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1103/PhysRevD.100.124005 http://cds.cern.ch/record/2663355 |
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